| dc.contributor.author | Schroder, K.P. | |
| dc.contributor.author | Napiwotzki, R. | |
| dc.contributor.author | Pauli, E.M. | |
| dc.date.accessioned | 2008-01-30T10:36:58Z | |
| dc.date.available | 2008-01-30T10:36:58Z | |
| dc.date.issued | 2005 | |
| dc.identifier.citation | Schroder , K P , Napiwotzki , R & Pauli , E M 2005 , A Model of the Local WD Population . in In: Procs of the 14th European Workshop on White Dwarfs - ASP Conference Series 334 . Astronomical Society of the Pacific , pp. 93-98 . | |
| dc.identifier.isbn | 1-58381-197-4 | |
| dc.identifier.isbn | 978-1-58381-268-6 | |
| dc.identifier.other | PURE: 171973 | |
| dc.identifier.other | PURE UUID: f3811768-b45b-4285-bb1f-8e4e339051dc | |
| dc.identifier.other | dspace: 2299/1442 | |
| dc.identifier.uri | http://hdl.handle.net/2299/1442 | |
| dc.description | Original paper can be found at: http://www.astrosociety.org/pubs/cs/328.html--Copyright Astronomical Society of the Pacific | |
| dc.description.abstract | We present a model of the solar neighbourhood (d<100 pc) white dwarf (WD) population and show its distribution in e®ective temperature and mass. The WDs are created by the death-rate of a population model matching the local stars observed by hipparcos, considering depletion as caused by the \thin disk" dynamics. | en |
| dc.language.iso | eng | |
| dc.publisher | Astronomical Society of the Pacific | |
| dc.relation.ispartof | In: Procs of the 14th European Workshop on White Dwarfs - ASP Conference Series 334 | |
| dc.title | A Model of the Local WD Population | en |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| dc.contributor.institution | School of Physics, Engineering & Computer Science | |
| dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
| dc.contributor.institution | Centre for Astrophysics Research | |
| rioxxterms.type | Other | |
| herts.preservation.rarelyaccessed | true | |
